Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10558
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dc.date.accessioned2017-04-19T12:54:52Zen
dc.date.available2017-04-19T12:54:52Zen
dc.date.issued2017-04-01en
dc.identifier.urihttp://hdl.handle.net/2122/10558en
dc.description.abstractManually scaled June noontime monthly median foE values at three European stations Rome, Juliusruh, and Slough/Chilton were used to understand the mechanism of foE long-term variations. The 11 year running mean smoothed foE manifests long-term (for some solar cycles) variations with the rising phase at the end of 1960–1985 and the falling phase after 1985. A close relationship (even in details) between (foEave)11y and (R12)11y variations with the correlation coefficient of 0.996 (absolutely significant according to Fisher F criterion) suggests that the Sun is the source of these (foEave)11y long-term variations. After removing solar activity long-term variations the residual (foEave)11y trend is very small (~0.029% per decade) being absolutely insignificant. This means that all (foEave)11y variations are removed with one solar activity index, (R12)11y, i.e., this means that long-term variations are fully controlled by solar activity. Theory of midlatitude daytime E region tells us that long-term variations of solar EUV in two lines λ = 977 Å (CIII) and λ = 1025.7 Å (HLyβ) and X-ray radiation with λ<100 Å (both manifesting the same long-term variations with the rising phase at the end of 1960–1985 and the falling phase after 1985) are responsible for the observed (foEave)11y variations. Therefore, the observed daytime midlatitude foE long-term variations have a natural (not anthropogenic) origin related to long-term variations of solar activity. No peculiarities in relation with the last deep solar minimum in 2008–2009 have been revealed.en
dc.language.isoEnglishen
dc.relation.ispartofJournal of Geophysical Research: Space Physicsen
dc.relation.ispartofseries4/122 (2017)en
dc.subjectMid-latitude foE long-term variations in ionosphere and thermosphereen
dc.titleA mechanism of midlatitude noontime foE long-term variations inferred from European observationsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber4466–4473en
dc.subject.INGVLong-term trend in the ionosphereen
dc.identifier.doi10.1002/2017JA023909en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeJCR Journalen
dc.contributor.authorMikhailov, Andreien
dc.contributor.authorPerrone, Loredanaen
dc.contributor.authorNusinov, A.en
dc.contributor.departmentPushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (IZMIRAN), Troitsk, Moscow Region 142190, Russiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptPushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (IZMIRAN), Troitsk, Moscow Region 142190, Russia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0003-4335-0345-
crisitem.author.orcid0000-0002-5171-0438-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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